Microwave Millisecond Spikes on July 30, 1997
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Abstract
The characteristics of the millisecond spikes with short durations and weak flux densities which were observed with high time resolution (1 ms)during a great type Ⅳ solar radio burst of 1990 July 30 are introduced.The time profiles of the spikes are statist ically analyzed and the parameters of the spike source are also estimated.
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